101 Helena

Last updated

101 Helena
Orbita asteroida 101.png
Orbital diagram
Discovery
Discovered by James Craig Watson
Discovery date15 August 1868
Designations
(101) Helena
Pronunciation /ˈhɛlənə/ [1]
Named after
Helen of Troy
A868 PA
Main belt
Orbital characteristics [2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 145.07 yr (52986 d)
Aphelion 2.94606  AU (440.724  Gm)
Perihelion 2.22353 AU (332.635 Gm)
2.58480 AU (386.681 Gm)
Eccentricity 0.13977
4.16 yr (1517.9 d)
Average orbital speed
18.44 km/s
236.265°
0° 14m 13.823s / day
Inclination 10.1976°
343.419°
348.030°
Earth  MOID 1.21369 AU (181.565 Gm)
Jupiter  MOID 2.4117 AU (360.79 Gm)
TJupiter 3.387
Physical characteristics
Dimensions 65.84±1.3  km [2]
Mass 3.0×1017 kg
Mean density
2.0 g/cm3
Equatorial surface gravity
0.0184 m/s2
Equatorial escape velocity
0.0348 km/s
23.080  h (0.9617  d) [2]
0.1898±0.008 [2]
Temperature ~173 K
S [3]
8.33

    101 Helena is a large, rocky main-belt asteroid. It was discovered by Canadian-American astronomer J. C. Watson on August 15, 1868, [4] and was named after Helen of Troy in Greek mythology.

    This object is orbiting the Sun with a period of 4.16 years and an eccentricity of 0.14. Its orbital plane is inclined by 10.2° to the plane of the ecliptic. Radar observations were made of this object on Oct 7 and 19, 2001 from the Arecibo Observatory. Analysis of the data gave an estimated ellipsoidal diameter of 71×63×63 ± 16% km. The mean diameter estimated from IRAS infrared measurements is 66 km, in agreement with the radar findings. It is classified as an S-type asteroid in the Tholen system, [3] [5] suggesting a predominantly silicate composition. 101 Helena is spinning on its axis with a period of 23 hours. [2]

    Related Research Articles

    <span class="mw-page-title-main">38 Leda</span> Main-belt asteroid

    38 Leda is a large, dark main-belt asteroid that was discovered by French astronomer J. Chacornac on January 12, 1856, and named after Leda, the mother of Helen of Troy in Greek mythology. In the Tholen classification system, it is categorized as a carbonaceous C-type asteroid, while the Bus asteroid taxonomy system lists it as a Cgh asteroid. The spectra of the asteroid displays evidence of aqueous alteration.

    <span class="mw-page-title-main">88 Thisbe</span> Main-belt asteroid

    88 Thisbe is the 13th largest main-belt asteroid. It was discovered by C. H. F. Peters on 15 June 1866, and named after Thisbe, heroine of a Roman fable. This asteroid is orbiting the Sun at a distance of 2.768 AU with a period of 4.60 years and an orbital eccentricity (ovalness) of 0.165. The orbital plane is inclined at an angle of 5.219° to the ecliptic.

    <span class="mw-page-title-main">109 Felicitas</span> Main-belt asteroid

    109 Felicitas is a dark and fairly large main-belt asteroid. It was discovered by German-American astronomer C. H. F. Peters on October 9, 1869, and named after Felicitas, the Roman goddess of success. The only observed stellar occultation by Felicitas is one from Japan.

    <span class="mw-page-title-main">111 Ate</span> Main-belt asteroid

    111 Ate is a main-belt asteroid discovered by the German-American astronomer C. H. F. Peters on August 14, 1870, and named after Ate, the goddess of mischief and destruction in Greek mythology. In the Tholen classification system, it is categorized as a carbonaceous C-type asteroid, while the Bus asteroid taxonomy system lists it as an Ch asteroid.

    <span class="mw-page-title-main">114 Kassandra</span> Main-belt asteroid

    114 Kassandra is a large and dark main-belt asteroid. It belongs to the rare class T. It was discovered by C. H. F. Peters on July 23, 1871, and is named after Cassandra, the prophetess in the tales of the Trojan War.

    <span class="mw-page-title-main">127 Johanna</span> Main-belt asteroid

    127 Johanna is a large, dark main-belt asteroid that was discovered by French astronomers Paul Henry and Prosper Henry on 5 November 1872, and is believed to be named after Joan of Arc. It is classified as a CX-type asteroid, indicating the spectrum shows properties of both a carbonaceous C-type asteroid and a metallic X-type asteroid.

    <span class="mw-page-title-main">137 Meliboea</span> Main-belt asteroid

    137 Meliboea is a large, dark main-belt asteroid that was discovered by Austrian astronomer J. Palisa at the Austrian Naval Observatory on 21 April 1874, the second of his many asteroid discoveries. It was later named after Meliboea, the daughter of Oceanus and Tethys in Greek mythology. The largest body in the Meliboea family of asteroids that share similar orbital elements, only 791 Ani approaches its size. It is classified as a C-type asteroid and may be composed of carbonaceous materials. The spectra of the asteroid displays evidence of aqueous alteration.

    <span class="mw-page-title-main">211 Isolda</span> Main-belt asteroid

    211 Isolda is a very large, dark main-belt asteroid. It is classified as a C-type asteroid and is probably composed of primitive carbonaceous material. The spectra of the asteroid displays evidence of aqueous alteration.

    <span class="mw-page-title-main">225 Henrietta</span> Main-belt asteroid

    225 Henrietta is a very large outer main-belt asteroid. It was discovered by Austrian astronomer Johann Palisa on April 19, 1882, in Vienna and named after Henrietta, wife of astronomer Pierre J. C. Janssen. The asteroid is orbiting at a distance of 3.39 AU from the Sun with a period of 6.24 years and an eccentricity (ovalness) of 0.26. The orbital plane is inclined at an angle of 20.9° to the plane of the ecliptic. 225 Henrietta belongs to Cybele group of asteroids and is probably in a 4:7 orbital resonance with the planet Jupiter.

    <span class="mw-page-title-main">247 Eukrate</span> Main-belt asteroid

    247 Eukrate is a rather large main-belt asteroid. It is dark and probably a primitive carbonaceous body. The asteroid was discovered by Robert Luther on March 14, 1885, in Düsseldorf. It was named after Eucrate, a Nereid in Greek mythology.

    <span class="mw-page-title-main">266 Aline</span> Main-belt asteroid

    266 Aline is a fairly large main belt asteroid that was discovered by Johann Palisa on 17 May 1887 in Vienna and is thought to have been named after the daughter of astronomer Edmund Weiss. It is a dark C-type asteroid and is probably composed of primitive carbonaceous material. 266 Aline is orbiting close to a 5:2 mean motion resonance with Jupiter, which is located at 2.824 AU.

    <span class="mw-page-title-main">270 Anahita</span> Main-belt asteroid

    270 Anahita is a stony S-type Main belt asteroid. It was discovered by C. H. F. Peters on October 8, 1887, in Clinton, New York, and was named after the Avestan divinity Aredvi Sura Anahita.

    <span class="mw-page-title-main">313 Chaldaea</span> Main-belt asteroid

    313 Chaldaea is a large Main belt asteroid. It is classified as a C-type asteroid and is probably composed of carbonaceous material. It was discovered by Johann Palisa on 30 August 1891 in Vienna. It was named in honor of the Chaldeans, considered the founders of astrology.

    <span class="mw-page-title-main">336 Lacadiera</span> Main-belt asteroid

    336 Lacadiera is a large Main belt asteroid. It is classified as a D-type asteroid and is probably composed of organic rich silicates, carbon and anhydrous silicates. The asteroid was discovered by Auguste Charlois on 19 September 1892 in Nice.

    <span class="mw-page-title-main">393 Lampetia</span> Main-belt asteroid

    393 Lampetia is a fairly large main belt asteroid that was discovered by German astronomer Max Wolf on 4 November 1894 in Heidelberg. It has an unusually low rotation rate, with a period estimated at 38.7 hours and a brightness variation of 0.14 in magnitude.

    405 Thia is a very large main-belt asteroid. It is classified as a C-type asteroid and is probably composed of carbonaceous material. This object was discovered by Auguste Charlois on July 23, 1895, in Nice, and was named after Theia, a Titaness in Greek mythology.

    429 Lotis is a large Main belt asteroid. It is classified as a probable C-type asteroid and is likely composed of primitive carbonaceous materials. This object was discovered by Auguste Charlois on 23 November 1897 in Nice.

    488 Kreusa is a C-type asteroid orbiting the Sun in the asteroid belt, with the type indicating a surface with a low albedo and high carbonaceous content. The spectra of the asteroid displays evidence of aqueous alteration.

    <span class="mw-page-title-main">505 Cava</span>

    505 Cava is a minor planet orbiting the Sun.

    622 Esther is a minor planet orbiting the Sun.

    References

    1. Noah Webster (1884) A Practical Dictionary of the English Language
    2. 1 2 3 4 5 Yeomans, Donald K., "101 Helena", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, archived from the original on 24 September 2014, retrieved 12 May 2016.
    3. 1 2 DeMeo, Francesca E.; et al. (2011), "An extension of the Bus asteroid taxonomy into the near-infrared" (PDF), Icarus, 202 (1): 160–180, Bibcode:2009Icar..202..160D, doi:10.1016/j.icarus.2009.02.005, archived from the original (PDF) on 17 March 2014, retrieved 22 March 2013. See appendix A.
    4. "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
    5. Magri, Christopher; Nolan, Michael C.; Ostro, Steven J.; Giorgini, Jon D. (January 2007), "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999 2003", Icarus, 186 (1): 126–151, Bibcode:2007Icar..186..126M, doi:10.1016/j.icarus.2006.08.018.